首页> 外文会议>International Astronautical Congress >PRECISE ATTITUDE ESTIMATION OF SOLAR SAIL SPACECRAFT UTILIZING COUPLING BETWEEN ATTITUDE AND ORBITAL DYNAMICS
【24h】

PRECISE ATTITUDE ESTIMATION OF SOLAR SAIL SPACECRAFT UTILIZING COUPLING BETWEEN ATTITUDE AND ORBITAL DYNAMICS

机译:利用姿态和轨道动力学耦合的太阳帆船的精确姿态估计

获取原文

摘要

Orbit determination is the process to estimate the position and velocity from a given set of observations of spacecraft. The common measurements used in orbit determination are range and range rate. For precise orbit determination, the acceleration of spacecraft by solar radiation pressure (SRP) must be taken into account. In order to incorporate the SRP acceleration, the attitude history and the SRP model - surface shape and optical surface feature of spacecraft - need to be known beforehand. Especially, in case of solar sail spacecraft, since their SRP effect is strong, coupling between attitude and orbital dynamics is more remarkable than ordinary ballistic missions. Therefore, by positively utilizing this coupling, it is possible to refine the attitude information based on the residual errors of orbit determination. In this study, we assume that the systematic errors in the orbit determination of the spacecraft are caused solely by the errors in attitude information, and propose an attitude error correction method which utilizes the coupling between attitude and orbital dynamics. In order to examine the validity of the method, the analysis of actual data is conducted. As actual data, flight data of IKAROS - Japanese interplanetary solar sail demonstration spacecraft - are used. The observations used in the orbit determination of IKAORS are range and range rate. In this paper, an estimator is designed whose input is the residuals of the orbit determination result - the difference between actual measurements and modelled observations of range and rage rate - and whose output is the amount of error correction in the attitude history. It is confirmed that orbit and attitude errors are both decreased through this method. This paper explains the theoretical background of this method and shows the result of analysis using the actual data.
机译:轨道确定是估计来自给定一组空间观察的位置和速度的过程。用于轨道测定的常见测量值是范围和范围率。为了精确轨道确定,必须考虑到太阳辐射压力(SRP)的航天器加速度。为了纳入SRP加速,姿态历史和SRP模型 - 表面形状和宇宙飞船的光学表面特征 - 需要预先已知。特别是,如果是太阳帆宇宙飞船,因为他们的SRP效果强,姿态和轨道动态之间的耦合比普通弹道特派团更显着。因此,通过阳性利用该耦合,可以基于轨道确定的残余误差来优化姿态信息。在这项研究中,我们假设航天器的轨道确定的系统误差仅通过姿态信息的误差来引起,并提出一种利用姿态和轨道动力学之间的耦合的姿态误差校正方法。为了检查该方法的有效性,进行实际数据的分析。作为实际数据,使用了ikaros的飞行数据 - 日本行星际太阳能风帆演示航天器。在轨道确定IKAORS的轨道中使用的观察是范围和范围率。在本文中,设计了估计器的输入是轨道确定结果的残差 - 实际测量和范围和愤怒率的建模观察之间的差异 - 其输出是姿态历史中的纠错量。确认轨道和姿态误差均通过该方法减少。本文介绍了该方法的理论背景,并使用实际数据显示了分析结果。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号